I read 1402.4119. I was even going to post it. It seemed to me that is was describing the "baby-steps" toward detecting dark matter.
The article reads to me to be self-admittedly non-definitive, but describes how we may able to detect the decay of dark matter as our abilities to measure it become more sophisticated, mentioning the future work of Astro-H as being the instrument by which we'll be able to validate the detections of current instruments.
I think the paper also mentions that there are a number of unidentified lines. I wonder what these will turn out to be.
One thing that I found "neat" was that the line was detected in the galaxies, but not in the "blank sky". So, clearly they're seeing something, but isn't dark matter everywhere, and hence, if decay can be seen in places where there is a lot of normal matter, wouldn't it be logical to say that the decay should also be able to be detected in the blank sky?
Or does dark matter tend to be more dense where there is normal matter? EDIT- Nevermind, I think I found the answer: DM Halos.
This was the first paper I learned of the "right-handed neutrino" being a DM candidate too.
For a guy that paid more attention to economics than cosmology, the arXiv website is A LOT of fun, and most educational.